Hostname: page-component-59f8fd8595-klmmf Total loading time: 0 Render date: 2023-03-21T19:18:11.975Z Has data issue: true Feature Flags: { "useRatesEcommerce": false } hasContentIssue true
  • English

HST Photometry of 47 Tucanae: Time Series Analysis and Search for Giant Planets

Published online by Cambridge University Press:  26 May 2016

Timothy M. Brown ,
David Charbonneau ,
Ronald L. Gilliland ,
M.D. Albrow ,
A. Burrows ,
W. D. Cochran ,
N. Baliber ,
P.D. Edmonds ,
S. Frandsen  and
S. Bruntt
...Show all authors
Timothy M. Brown
Affiliation:
High Altitude Observatory/National Center for Atmospheric Research, 3450 Mitchell Lane, Boulder, CO 80303, USA
David Charbonneau
Affiliation:
HAO/NCAR and Harvard/Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Ronald L. Gilliland
Affiliation:
Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218, USA
M.D. Albrow
Affiliation:
STScI
A. Burrows
Affiliation:
U. Arizona
W. D. Cochran
Affiliation:
U. Texas
N. Baliber
Affiliation:
U. Texas
P.D. Edmonds
Affiliation:
SAO
S. Frandsen
Affiliation:
U. Aarhus
S. Bruntt
Affiliation:
U. Aarhus
P. Guhathakurta
Affiliation:
UCSC
P. Choi
Affiliation:
UCSC
D.N.C. Lin
Affiliation:
UCSC
S.S. Vogt
Affiliation:
UCSC
G.W. Marcy
Affiliation:
UCB
M. Mayor
Affiliation:
Obs. Geneva
D. Naef
Affiliation:
Obs. Geneva
E. F. Milone
Affiliation:
U. Calgary
C. R. Stagg
Affiliation:
U. Calgary
M.D. Williams
Affiliation:
U. Calgary
A. Sarajedini
Affiliation:
Wesleyan U.
S. Sigurdsson
Affiliation:
PSU
D.A. VandenBerg
Affiliation:
U. Victoria

Abstract

HTML view is not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Gilliland et al. (2000) have reported HST photometric observations of 34000 stars in the globular cluster 47 Tuc, showing an absence of close-in giant planets in that cluster relative to their frequency in the solar neighborhood. Here we describe the methods of time-series analysis that were used to search the 47 Tuc data for transits by giant extrasolar planets, and the means by which these methods were validated.

Type
Part I: Discovery and study of extrasolar planets - current
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 66 - 68
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Brown, T.M. et al. 2001, ApJ (in preparation).Google Scholar
Brown, T.M., Charbonneau, D., Gilliland, R.L., Noyes, R.W., & Burrows, A. 2001, ApJ (submitted).Google Scholar
Charbonneau, D., Brown, T.M., Latham, D.W., & Mayor, M. 2000, ApJ 529, L45.CrossRefGoogle Scholar
Gilliland, R.L. et al. 2000, ApJ (in press).Google Scholar
Henry, G.W., Marcy, G.W., Butler, R.P., & Vogt, S.S. 2000, ApJ 529, L41.CrossRefGoogle Scholar
Jenkins, J.M., Doyle, L.R., & Cullers, D.K. 1996, Icarus 119, 244.CrossRefGoogle Scholar
Marcy, G.W., Cochran, W.D. & Mayor, M. 2000, in Protostars and Planets IV, ed. Mannings, V., Boss, A.P. & Russell, S., (Tucson: University of Arizona Press), 1285.Google Scholar